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1545 Thernöe

From Wikipedia, the free encyclopedia
Elongated main-belt asteroid

1545 Thernöe
Shape model of Thernöe from itslightcurve
Discovery[1]
Discovered byL. Oterma
Discovery siteTurku Obs.
Discovery date15 October 1941
Designations
(1545) Thernöe
Named after
Karl August Thernöe
(Danish astronomer)[2]
1941 UW · 1932 YD
1955 VV · 1957 HY
A906 FE · A915 CE
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc111.21 yr (40,619 days)
Aphelion3.4299AU
Perihelion2.1097 AU
2.7698 AU
Eccentricity0.2383
4.61yr (1,684 days)
84.917°
0° 12m 49.68s / day
Inclination2.9542°
51.800°
90.542°
Physical characteristics
16.12±5.02 km[4]
17.796±0.210 km[5]
18.656±0.376 km[6]
18.71±1.1 km[7]
19.37±0.31 km[8]
17.20±0.01 h[9]
17.20321±0.0001 h[10]
0.092±0.004[8]
0.0962±0.013[7]
0.097±0.012[6]
0.1063±0.0153[5]
0.13±0.10[4]
SMASS =K[1] · C[11]
11.76[4] · 11.8[11][5][6][7][8] · 11.9[1] · 12.09±0.45[12]

1545 Thernöe (provisional designation1941 UW) is an elongatedbackground asteroid from the central region of theasteroid belt. It was discovered on 15 October 1941, by Finnish astronomerLiisi Oterma atTurku Observatory in Southwest Finland.[3] The uncommonK-type asteroid has arotation period of 16.1 hours and measures approximately 18 kilometers (11 miles) in diameter. It was later named after Danish astronomerKarl August Thernöe.[2]

Orbit

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Thernöe orbits the Sun in thecentral main-belt at a distance of 2.1–3.4 AU once every 4 years and 7 months (1,684 days). Its orbit has aneccentricity of 0.24 and aninclination of 3° with respect to theecliptic.[1] It was first identified asA906 FE atHeidelberg Observatory in 1906, extending the body'sobservation arc by 35 years prior to its official discovery observation at Turku.[3]

Naming

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Thisminor planet was named after Karl August Thernöe (1911–1987), Danish astronomer and celestial mechanic atØstervold Observatory in Copenhagen. He was also a popularizer of astronomy and director ofIAU'sCentral Bureau for Astronomical Telegrams during 1950–1964.[2][13] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3930).[14]

Physical characteristics

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Spectral type

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In theSMASS taxonomy, Thernöe is classified as a rareK-type asteroid, a newly introduced subtype that belongs to the broaderS-complex of stony bodies.[1] Conversely, CALL groups Thernöe into the carbonaceousC-complex.[11]

Rotation period and pole

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In December 2006, a rotationallightcurve of Thernöe was obtained from photometric observations by French amateur astronomerRené Roy. Lightcurve analysis gave a well-definedrotation period of 17.20 hours with a brightness variation of 0.76magnitude (U=3).[9] The high lightcurve-amplitude of 0.76 indicates that the body has a non-spheroidal shape.

A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database, gave a concurring period of 17.20321 hours, as well as aspin axis of (164.0°, −5.0°) inecliptic coordinates (λ, β).[10]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Thernöe measures between 16.12 and 19.37 kilometers in diameter and its surface has analbedo between 0.092 and 0.13.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link (CALL) adopts the results obtained by IRAS, that is, an albedo of 0.0962 and diameter of 18.71 kilometers with anabsolute magnitude of 11.8.[11]

References

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  1. ^abcdefg"JPL Small-Body Database Browser: 1545 Thernoe (1941 UW)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1545) Thernöe".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 122.doi:10.1007/978-3-540-29925-7_1546.ISBN 978-3-540-00238-3.
  3. ^abc"1545 Thernoe (1941 UW)".Minor Planet Center. Retrieved3 April 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  5. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 35447010.
  6. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.S2CID 46350317. Retrieved3 April 2017.
  7. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  8. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1545) Thernöe".Geneva Observatory. Retrieved3 April 2017.
  10. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573.S2CID 118427201. Retrieved3 April 2017.
  11. ^abcd"LCDB Data for (1545) Thernöe". Asteroid Lightcurve Database (LCDB). Retrieved3 April 2017.
  12. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved3 April 2017.
  13. ^Erik Høg (7 December 2016). "Young astronomer in Denmark 1946 to 1958".Nuncius Hamburgensis.38.arXiv:1512.01924.Bibcode:2015arXiv151201924H.
  14. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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